papers

Publications (20)

astro-ph.GA2023

MusE GAs FLOw and Wind (MEGAFLOW) X. The cool gas and covering fraction of MgII in galaxy groups

Maxime Cherrey, Nicolas Bouché, Johannes Zabl +8

We present a study of the cool gas ( K) traced by MgII absorptions around groups of galaxies in the MEGAFLOW survey. Using a combination of two algorithms we blindly…

astro-ph.GA2017

The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection

Roland Bacon, Simon Conseil, David Mary +24

We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering 90\% of the entire HUDF region with a 10-hour deep exposure time, plus a deeper 31-hour exposure…

astro-ph.CO2014

SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4

Fernando Buitrago, Christopher J. Conselice, Benoit Epinat +3

There is cumulative evidence showing that, for the most massive galaxies, the fraction of disk-like objects compared to those with spheroidal properties increases with redshift. Ho…

astro-ph.GA2022

The MUSE Hubble Ultra Deep Field surveys: Data release II

Roland Bacon, Jarle Brinchmann, Simon Conseil +30

We present the second data release of the MUSE Hubble UDF surveys, which includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D content, amazing dep…

astro-ph.GA2017

Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7

Mark Swinbank, Chris Harrison, James Trayford +23

We present a MUSE and KMOS dynamical study 405 star-forming galaxies at redshift z=0.28-1.65 (median redshift z=0.84). Our sample are representative of star-forming, main-sequence…

astro-ph.GA2018

GHASP: an H kinematical survey of spiral galaxies - XI. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using WISE photometry

Marie Korsaga, Claude Carignan, Philippe Amram +2

We present the mass distribution of a sample of 121 nearby galaxies with high quality optical velocity fields and available infra-red 3.4 m data. Contrary to previo…